Formation of electron radiation belts at Saturn by Z-mode wave acceleration
Radial diffusion is the only mechanism considered to accelerate trapped electrons to relativistic energies in Saturn’s magnetic field, forming radiation belts.
E. E. Woodfield +5 more
doaj +1 more source
A Past Episode of Rapid Tidal Evolution of Enceladus? [PDF]
Matija Ćuk, Maryame El Moutamid
openalex +1 more source
Analysis of Enceladus’s Time-variable Space Environment to Magnetically Sound its Interior
We provide a comprehensive study of Enceladus’s time-variable magnetic field environment and identify in measurements of the Cassini spacecraft signatures that appear to be consistent with induced fields from the moon’s interior.
Joachim Saur +3 more
doaj +1 more source
Low Energy Subsurface Environments as Extraterrestrial Analogs
Earth’s subsurface is often isolated from phototrophic energy sources and characterized by chemotrophic modes of life. These environments are often oligotrophic and limited in electron donors or electron acceptors, and include continental crust ...
Rose M. Jones +2 more
doaj +1 more source
Curtain-based Maps of Eruptive Activity in Enceladus’s South-polar Terrain at 15 Cassini Epochs
We map surface eruptive activity in Cassini images of Enceladus’s south-polar terrain (SPT) at 15 epochs spanning late 2009 to late 2015 using a refined curtain approach derived from that of J. N. Spitale et al. (S2015).
Joseph N. Spitale +5 more
doaj +1 more source
Cryoclastic origin of particles on the surface of Enceladus [PDF]
W. Degruyter, Michael Manga
openalex +1 more source
Microwaving Saturn's airless icy moons Mimas, Enceladus, Tethys, Dione, Rhea, Iapetus and Phoebe
Alice Le Gall +4 more
openalex +1 more source
Exploring the Interior Structure and Mode of Tidal Heating in Enceladus
Enceladus is among the most intriguing bodies in the solar system due to its astrobiological potential. Determining the extent and duration of habitability (i.e., sustained habitability ) requires characterizing the interior properties and the level and ...
Amirhossein Bagheri +6 more
doaj +1 more source
Orbital evolution of Saturn’s mid-sized moons and the tidal heating of Enceladus [PDF]
Ayano Nakajima +3 more
openalex +1 more source
Impacts on Ocean Worlds Are Sufficiently Frequent and Energetic to Be of Astrobiological Importance
Evidence for the beneficial role of impacts in the creation of urable or habitable environments on Earth prompts the question of whether meteorite impacts could play a similar role at other potentially urable/habitable worlds like Enceladus, Europa, and ...
Shannon M. MacKenzie +14 more
doaj +1 more source

